Template:Solar Saros series 146
This eclipse is a part of Saros series 146, repeating every 18 years, 11 days, and containing 76 events. The series started with a partial solar eclipse on September 19, 1541. It contains total eclipses from May 29, 1938 through October 7, 2154; hybrid eclipses from October 17, 2172 through November 20, 2226; and annular eclipses from November 30, 2244 through August 10, 2659. The series ends at member 76 as a partial eclipse on December 29, 2893. Its eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.
The longest duration of totality was produced by member 26 at 5 minutes, 21 seconds on June 30, 1992, and the longest duration of annularity will be produced by member 63 at 3 minutes, 30 seconds on August 10, 2659. All eclipses in this series occur at the Moon’s descending node of orbit.[1]
| Series members 16–37 occur between 1801 and 2200: | ||
|---|---|---|
| 16 | 17 | 18 |
 March 13, 1812 |
 March 24, 1830 |
 April 3, 1848 |
| 19 | 20 | 21 |
 April 15, 1866 |
 April 25, 1884 |
 May 7, 1902 |
| 22 | 23 | 24 |
 May 18, 1920 |
 May 29, 1938 |
 June 8, 1956 |
| 25 | 26 | 27 |
 June 20, 1974 |
 June 30, 1992 |
 July 11, 2010 |
| 28 | 29 | 30 |
 July 22, 2028 |
 August 2, 2046 |
 August 12, 2064 |
| 31 | 32 | 33 |
 August 24, 2082 |
 September 4, 2100 |
 September 15, 2118 |
| 34 | 35 | 36 |
 September 26, 2136 |
 October 7, 2154 |
 October 17, 2172 |
| 37 | ||
 October 29, 2190 | ||
References
- ^ "NASA - Catalog of Solar Eclipses of Saros 146". eclipse.gsfc.nasa.gov.